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dc.contributor.authorVandaele, A.C.
dc.contributor.authorMahieux, A.
dc.contributor.authorRobert, S.
dc.contributor.authorBerkenbosch, S.
dc.contributor.authorClairquin, R.
dc.contributor.authorDrummond, R.
dc.contributor.authorLetocart, V.
dc.contributor.authorNeefs, E.
dc.contributor.authorRistic, B.
dc.contributor.authorWilquet, V.
dc.contributor.authorColomer, F.
dc.contributor.authorBelyaev, D.
dc.contributor.authorBertaux, J.-L.
dc.date2013
dc.date.accessioned2016-03-25T11:11:11Z
dc.date.available2016-03-25T11:11:11Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2927
dc.descriptionThe SOIR instrument on board the ESA Venus Express mission has been operational since the insertion of the satellite around Venus in April 2006. Since then, it has delivered high quality IR solar occultation spectra of the atmosphere of Venus. The different steps from raw spectra to archived data are described and explained in detail here. These consist of corrections for the dark current and for the non-linearity of the detector; removing bad pixels, as well as deriving noise. The spectral calibration procedure is described, along with all ancillary data necessary for the understanding and interpretation of the SOIR data. These include the full characterization of the AOTF filter, one of the major elements of the instrument. All these data can be found in the ESA PSA archive.
dc.languageeng
dc.titleImproved calibration of SOIR/Venus Express spectra
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeAncillary data
dc.subject.freeArchived data
dc.subject.freeBad pixels
dc.subject.freeHigh quality
dc.subject.freeMajor elements
dc.subject.freeSolar occultation
dc.subject.freeSpectral calibration
dc.subject.freeVenus express mission
dc.subject.freeOptical constants
dc.subject.freeOptics
dc.source.titleOptics Express
dc.source.volume21
dc.source.issue18
dc.source.page21148-21161
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/OE.21.021148
dc.identifier.scopus2-s2.0-84884541774


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